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(XRD) for structural analysis; • Dynamic light scattering (DLS) for particle size distribution and colloidal stability; • Magnetometry techniques (e.g., VSM, SQUID) for magnetic property evaluation
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integrity, uniform pressure distribution, and efficient thermal management under high-temperature operational conditions (500-1000 °C); 2. Implement and validate an advanced computational framework
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for fitting spectral energy distributions (SED-fitting), to analyze thousands of galaxies within the survey’s coverage area. We seek an astronomer with experience in extragalactic astrophysics to explore
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